Mapping for nonlinear electron interaction with whistler-mode waves

被引:20
作者
Artemyev, A. V. [1 ,3 ]
Neishtadt, A. I. [2 ,3 ]
Vasiliev, A. A. [3 ]
机构
[1] Univ Calif Los Angeles, Inst Geophys & Planetary Phys, Los Angeles, CA 90095 USA
[2] Loughborough Univ, Dept Math Sci, Loughborough LE11 3TU, Leics, England
[3] Russian Acad Sci IKI, Space Res Inst, 84-32 Profsoyuznaya Str, Moscow 117997, Russia
基金
美国国家科学基金会; 俄罗斯科学基金会;
关键词
OUTER RADIATION BELT; PARTICLE INTERACTIONS; BEAM INTERACTION; LOCAL ACCELERATION; MAGNETIC-FIELD; CHORUS WAVES; VLF WAVES; OBLIQUE; RESONANCE; SPACE;
D O I
10.1063/1.5144477
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
The resonant interaction of relativistic electrons and whistler-mode waves is an important mechanism of electron acceleration and scattering in the Earth radiation belts and other space plasma systems. For low amplitude waves, such an interaction is well described by the quasi-linear diffusion theory, whereas nonlinear resonant effects induced by high-amplitude waves are mostly investigated (analytically and numerically) using the test particle approach. In this paper, we develop a mapping technique for the description of this nonlinear resonant interaction. Using the Hamiltonian theory for resonant systems, we derive the main characteristics of electron transport in the phase space and combine these characteristics to construct the map. This map can be considered as a generalization of the classical Chirikov map for systems with nondiffusive particle transport and allows us to model the long-term evolution of the electron distribution function.
引用
收藏
页数:12
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